On the origin of the inertia: the modified Newtonian dynamics theory

The sameness between the inertial mass and the gravitational mass is an assumption and not a consequence of the equivalent principle is shown. In the context of the Sciama’s inertia theory, the sameness between the inertial mass and the gravitational mass is discussed and a certain condition which must be experimentally satisfied is given. The inertial force proposed by Sciama, in a simple case, is derived from the Assis’ inertia theory based in the introduction of a Weber type force. The origin of the inertial force is totally justified taking into account that the Weber force is, in fact, an approximation of a simple retarded potential, see [18, 19]. The way how the inertial forces are also derived from some solutions of the general relativistic equations is presented. We wonder if the theory of inertia of Assis is included in the framework of the General Relativity. In the context of the inertia developed in the present paper we establish the relation between the constant acceleration a0 , that appears in the classical Modified Newtonian Dynamics (M0ND) theory, with the Hubble constant H0 , i.e. a0 ≈ cH0 .

Estados expulsores y semipersonas en la Unión Europea

La aprobación en junio de 2008 por el Parlamento Europeo de la Directiva de retorno —denominada también Directiva de la infamia o Directiva de expulsión— consolida el proceso de involución que sobre los derechos humanos se viene produciendo en la Unión Europea desde que el miedo a la inmigración irregular se incardinó en sus instituciones. Si bien las legislaciones de extranjería de los años ochenta contenían normas que regulaban el internamiento y la expulsión no es hasta la Directiva 2001/40/CE que comienza a tomar forma una política comunitaria centrada en la inmigración irregular y las expulsiones de migrantes. Las medidas de retorno son, dice la Comisión europea, “una piedra angular de la política de migración de la UE”. Desde entonces, la barbarie de los centros de retención e internamiento, el socavamiento de los derechos y la exclusión y criminalización de los migrantes extranjeros se han convertido en el caballo de batalla de las asociaciones defensoras de los derechos humanos. La erosión que las legislaciones y medidas de expulsión están provocado en los derechos y libertades y en las instituciones del Estado de derecho es inmensa. El retroceso y la erosión en los derechos y libertades es tan grande que ya no es posible continuar hablando sin más de Estados de derecho en la UE, sino más bien de máquinas administrativas para el internamiento y la expulsión, de “Estados expulsores” (1), donde las personas extranjeras son tratadas como semipersonas (2) e incluso como “no-personas” (3).

Estados expulsores y semipersonas en la Unión Europea

La aprobación en junio de 2008 por el Parlamento Europeo de la Directiva de retorno —denominada también Directiva de la infamia o Directiva de expulsión— consolida el proceso de involución que sobre los derechos humanos se viene produciendo en la Unión Europea desde que el miedo a la inmigración irregular se incardinó en sus instituciones. Si bien las legislaciones de extranjería de los años ochenta contenían normas que regulaban el internamiento y la expulsión no es hasta la Directiva 2001/40/CE que comienza a tomar forma una política comunitaria centrada en la inmigración irregular y las expulsiones de migrantes. Las medidas de retorno son, dice la Comisión europea, “una piedra angular de la política de migración de la UE”. Desde entonces, la barbarie de los centros de retención e internamiento, el socavamiento de los derechos y la exclusión y criminalización de los migrantes extranjeros se han convertido en el caballo de batalla de las asociaciones defensoras de los derechos humanos. La erosión que las legislaciones y medidas de expulsión están provocado en los derechos y libertades y en las instituciones del Estado de derecho es inmensa. El retroceso y la erosión en los derechos y libertades es tan grande que ya no es posible continuar hablando sin más de Estados de derecho en la UE, sino más bien de máquinas administrativas para el internamiento y la expulsión, de “Estados expulsores”(1), donde las personas extranjeras son tratadas como semipersonas (2) e incluso como“no-personas” (3).

Supergravity models of (3+1)-dimensional QCD

The most general black M5-brane solution of eleven-dimensional supergravity (with a flat R4 spacetime in the brane and a regular horizon) is characterized by charge, mass and two angular momenta. We use this metric to construct general dual models of large-N QCD (at strong coupling) that depend on two free parameters. The mass spectrum of scalar particles is determined analytically (in the WKB approximation) and numerically in the whole two-dimensional parameter space. We compare the mass spectrum with analogous results from lattice calculations, and find that the supergravity predictions are close to the lattice results everywhere on the two dimensional parameter space except along a special line. We also examine the mass spectrum of the supergravity Kaluza-Klein (KK) modes and find that the KK modes along the compact D-brane coordinate decouple from the spectrum for large angular momenta. There are however KK modes charged under a U(1)×U(1) global symmetry which do not decouple anywhere on the parameter space. General formulas for the string tension and action are also given.

Large N QCD from rotating branes

We study large N SU(N) Yang-Mills theory in three and four dimensions using a one-parameter family of supergravity models which originate from non-extremal rotating D-branes. We show explicitly that varying this angular momentum parameter decouples the Kaluza-Klein modes associated with the compact D-brane coordinate, while the mass ratios for ordinary glueballs are quite stable against this variation, and are in good agreement with the latest lattice results. We also compute the topological susceptibility and the gluon condensate as a function of the "angular momentum" parameter.

The first SEPServer event catalogue 68-MeV solar proton events observed at 1 AU in 1996-2010

SEPServer is a three-year collaborative project funded by the seventh framework programme (FP7-SPACE) of the European Union. The objective of the project is to provide access to state-of-the-art observations and analysis tools for the scientific community on solar energetic particle (SEP) events and related electromagnetic (EM) emissions. The project will eventually lead to better understanding of the particle acceleration and transport processes at the Sun and in the inner heliosphere. These processes lead to SEP events that form one of the key elements of space weather. In this paper we present the first results from the systematic analysis work performed on the following datasets: SOHO/ERNE, SOHO/EPHIN, ACE/EPAM, Wind/WAVES and GOES X-rays. A catalogue of SEP events at 1 AU, with complete coverage over solar cycle 23, based on high-energy (~68-MeV) protons from SOHO/ERNE and electron recordings of the events by SOHO/EPHIN and ACE/EPAM are presented. A total of 115 energetic particle events have been identified and analysed using velocity dispersion analysis (VDA) for protons and time-shifting analysis (TSA) for electrons and protons in order to infer the SEP release times at the Sun. EM observations during the times of the SEP event onset have been gathered and compared to the release time estimates of particles. Data from those events that occurred during the European day-time, i.e., those that also have observations from ground-based observatories included in SEPServer, are listed and a preliminary analysis of their associations is presented. We find that VDA results for protons can be a useful tool for the analysis of proton release times, but if the derived proton path length is out of a range of 1 AU < s[3 AU, the result of the analysis may be compromised, as indicated by the anti-correlation of the derived path length and release time delay from the asso ciated X-ray flare. The average path length derived from VDA is about 1.9 times the nominal length of the spiral magnetic field line. This implies that the path length of first-arriving MeV to deka-MeV protons is affected by interplanetary scattering. TSA of near-relativistic electrons results in a release time that shows significant scatter with respect to the EM emissions but with a trend of being delayed more with increasing distance between the flare and the nominal footpoint of the Earth-connected field line.

Filmipäällystimen nippitapahtuman vaikutus päällystyskoneen ajettavuuteen

Työn tavoitteena oli syventyä filmipäällystimen nippitapahtumaan ja siellä tapahtuviin ilmiöihin. Tämän lisäksi selvitettiin esipäällystysparametrien ja pohjapaperin merkitys filmipäällystimen ajettavuudelle. Erityisesti pyrittiin selvittämään päällystemäärän ja applikointitelojen momenttieron vaikutus ajettavuuteen sekä kiihdytysvaiheessa ilmenevien ajettavuusongelmien syntymekanismit. Työn kokeellinen osa jakaantui kahteen osaan. Ensimmäisessä osassa pyritään löytämään lisäymmärrystä nippitapahtuman ilmiöille joita sitten hyödynnetään toisen osan koeajoissa. Staattisilla kuormituskokeilla tutkittiin telapinnan kokoonpuristumista ja suurnopeus-kamerakuvauksilla nipin geometriaa päällystyskoneen ajon aikana. Applikointitelojen momenttierokoeajoilla pyrittiin selvittämään paperiradan mahdollista luistoa nipissä. MCA-kosteuspitoisuusanalysaattorilla mitattiin nippitapahtuman muutosten vaikutusta filmipäällystimen paluufilmin ominaisuuksiin. Muuttelemalla päällystemäärää ja – jakaumaa sekä applikointitelojen momenttieroa selvitettiin esipäällystysparametrien vaikutus filmipäällystimen ajettavuuteen. Muokkaamalla pohjapaperin absorptiokykyä sekä pastan vedenpidätyskykyä tutkittiin nestepenetraation vaikutusta ajettavuuteen. Telapinnan kokoonpuristuman havaittiin olevan pieni eikä ajon aikana nipin geometriassa havaittu muutoksia. Paperiradan todettiin luistavan nipissä, mutta luistoilmiö oli huomattavasti pienempi mitä nopeuserolukemista voidaan päätellä. Kiihdytysvaiheessa havaittiin selviä muutoksia paluufilmissä, mutta ajon aikana paluufilmi pysyi lähes vakiona. Päällystemäärän todettiin olevan suurin yksittäinen tekijä filmipäällystimen ajettavuudessa ja siihen tulee kiinnittää erityistä huomiota filmipäällystimen kiihdytysvaiheessa. Aukirullauksen levitystelan vaihdon myötä todettiin pohjapaperiin kohdistuvilla kuormituksilla olevan myös suuri merkitys filmipäällystimen ajettavuudelle.

Spectral energy distribution of the gamma-ray microquasar LS 5039

The microquasar LS 5039 has recently been detected as a source of very high energy (VHE) $\gamma$-rays. This detection, that confirms the previously proposed association of LS 5039 with the EGRET source 3EG~J1824$-$1514, makes of LS 5039 a special system with observational data covering nearly all the electromagnetic spectrum. In order to reproduce the observed spectrum of LS 5039, from radio to VHE $\gamma$-rays, we have applied a cold matter dominated jet model that takes into account accretion variability, the jet magnetic field, particle acceleration, adiabatic and radiative losses, microscopic energy conservation in the jet, and pair creation and absorption due to the external photon fields, as well as the emission from the first generation of secondaries. The radiative processes taken into account are synchrotron, relativistic Bremsstrahlung and inverse Compton (IC). The model is based on a scenario that has been characterized with recent observational results, concerning the orbital parameters, the orbital variability at X-rays and the nature of the compact object. The computed spectral energy distribution (SED) shows a good agreement with the available observational data.

Phyllochron estimation in intercropped strawberry and monocrop systems in a protected environment

The phyllochron is defined as the time required for the appearance of successive leaves on a plant; this characterises plant growth, development and adaptation to the environment. To check the growth and adaptation in cultivars of strawberry grown intercropped with fig trees, it was estimated the phyllochron in these production systems and in the monocrop. The experiment was conducted in greenhouses at the University of Passo Fundo (28º15'41'' S, 52º24'45'' W and 709 m) from June 8th to September 4th, 2009; this comprised the period of transplant until the 2nd flowering. The cultivars Aromas, Camino Real, Albion, Camarosa and Ventana, which seedlings were originated from the Agrícola LLahuen Nursery in Chile, as well as Festival, Camino Real and Earlibrite, originated from the Viansa S.A. Nursery in Argentina, were grown in white polyethylene bags filled with commercial substrate (Tecnomax®) and evaluated. The treatments were arranged in a randomised block design and four replicates were performed. A linear regression was realized between the leaf number (LN) in the main crown and the accumulated thermal time (ATT). The phyllochron (degree-day leaf-1) was estimated as the inverse of the angular coefficient of the linear regression. The data were submitted to ANOVA, and when significance was observed, the means were compared using the Tukey test (p < 0.05). The mean and standard deviation of phyllochrons of strawberry cultivars intercropped with fig trees varied from 149.35ºC day leaf-1 ± 31.29 in the Albion cultivar to 86.34ºC day leaf-1 ± 34.74 in the Ventana cultivar. Significant differences were observed among cultivars produced in a soilless environment with higher values recorded for Albion (199.96ºC day leaf-1 ± 29.7), which required more degree-days to produce a leaf, while cv. Ventana (85.76ºC day leaf-1 ± 11.51) exhibited a lower phyllochron mean value. Based on these results, Albion requires more degree-days to issue a leaf as compared to cv. Ventana. It was conclude that strawberry cultivars can be grown intercropped with fig trees (cv. Roxo de Valinhos).

Seleção de modelos de regressão para estimar a área foliar de macieiras 'Royal gala' e 'Fuji suprema' sob tela antigranizo e em céu aberto

O objetivo deste trabalho foi ajustar e testar modelos matemáticos simples, precisos e acurados para estimar a área foliar de macieiras 'Royal Gala' e 'Fuji Suprema' cultivadas sob tela antigranizo e em céu aberto. O experimento foi conduzido em pomar comercial no município de Vacaria-RS, nos ciclos vegetativos de 2008/2009 e 2009/2010. Equações de regressão linear e quadrática foram ajustadas para estimativa da área foliar em função das dimensões das folhas. A seleção dos melhores modelos baseou-se no quadrado médio do erro, no coeficiente de determinação, no erro-padrão da estimativa e na significância dos coeficientes das equações. A área foliar estimada pelos melhores modelos foi comparada com dados obtidos de medição por planímetro e estimados por fotografias digitais. A prova dos modelos baseou-se na significância do coeficiente angular, na linha 1:1 e na raiz quadrada do quadrado médio do erro. Modelos linear e quadrático que consideram o comprimento e a largura das folhas estimam com acurácia e precisão a área foliar de macieiras 'Royal Gala' e 'Fuji Suprema', tanto sob tela antigranizo quanto em céu aberto. A área foliar de macieira estimada por modelos de regressão que utilizam comprimento e largura de folhas é similar à obtida por planímetro ou fotografia digital.

Sähköisen lineaariservomoottorijärjestelmän dynamiikan simulointi

Työssä johdettiin sähköisen lineaariservomoottorijärjestelmän dynaaminen malli. Lineaarimoottori on keksintönä vanha, mutta vasta viimeaikoina kestomagneettimateriaalien kehittyessä ja halvetessa lineaarimoottorista on tullut varteenotettava vaihtoehto pyörivän moottorin ja lineaarisen liikkeen toteuttavan mekanismin yhdistelmälle. Kestomagnetoituja lineaarimoottoreita käytetään sovelluksissa, joissa tarvitaan tarkkaa paikoitusta ja nopeudella ja kiihtyvyydellä on suuret vaatimukset. Moottorimalli toteutettiin vuorovaikutteisena simulointimallina. Moottorimalli, josta saatiin moottorin voima, rakennettiin MatLabâ 6.0/Simulinkâ –ohjelmalle ja moottoriin kiinnitetyn mekaniikan malli ADAMS 10.0 –ohjelmalle. Mallit on liitetty tämän jälkeen vuorovaikutteiseksi simulointimalliksi. Simuloinnista saatuja tuloksia on verrattu koneautomaation laboratorioon hankitun lineaarimoottorijärjestelmän mitattuihin vasteisiin.

Observation of VHE γ-rays from Cassiopeia A with the MAGIC telescope

Aims:We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A Methods: The shell-type supernova remnant Cassiopeia A was observed with the 17 m MAGIC telescope between July 2006 and January 2007 for a total time of 47 h. Results: The source was detected above an energy of 250 GeV with a significance of 5.2σ and a photon flux above 1 TeV of (7.3 ± 0.7_stat ± 2.2_sys) × 10-13 cm-2s-1. The photon spectrum is compatible with a power law dN/dE ∝ E-Γ with a photon index Γ = 2.3 ± 0.2_stat ± 0.2_sys. The source is point-like within the angular resolution of the telescope.

Moottoriajoneuvon suorituskyvyn mittausjärjestelmä

Työn tarkoituksena oli toteuttaa moottoriajoneuvon suorituskyvyn mittaukseen käytettävä järjestelmä. Järjestelmä koostuu sylinterin muotoisesta rullasta ja tiedonkeruujärjestelmästä. Rullaa, jonka hitausmomentti tunnetaan kiihdytetään ajoneuvon vetopyörien välityksellä ja mitatuista arvoista lasketaan teho ja vääntömomenttiarvot moottorin kierrosluvun funktiona. Tiedonkeruu tapahtuu PC-mikrotietokoneen avulla, johon on liitetty tiedonkeruukortti. PC-mikrotietokone muodostaa käyttöliittymän, jonka avulla saadut tulokset esitetään kuvaajien avulla käyttäjälle. Käyttöliittymän avulla suoritetaan myös tulosten talletus ja raportin tulostus. Teoriaosassa tarkastellaan suorituskyvyn mittaamiseen käytettyjä menetelmiä ja laitteistoja, sekä tiedonkeruujärjestelmän rakennetta ja sen valintaan vaikuttavia tekijöitä. Käytännön osassa suunnitellaan muokkainkortti, jonka avulla erilaisilta antureilta saadut signaalit voidaan sovittaa tiedonkeruukortin tuloalueelle sopiviksi. Myös käyttöliittymän toimintaa ja sen rakentamiseen käytettyjä työkaluja tarkastellaan.

Behavior of propagating and evanescent components in azimuthally polarized non-paraxial fields

The contribution of the propagating and the evanescent waves associated with freely propagating non-paraxial light fields whose transverse component is azimuthally polarized at some plane is investigated. Analytic expressions are derived for describing both the spatial shape and the relative weight of the propagating and the evanescent components integrated over the transverse plane. The analysis is carried out within the framework of the plane-wave angular spectrum approach. These results are used to illustrate the behavior of a kind of donut-like beams with transverse azimuthal polarization at some plane.

Synergies between optical and physical variables in intercepting parabolic targets.

Interception requires precise estimation of time-to-contact (TTC) information. A long-standing view posits that all relevant information for extracting TTC is available in the angular variables, which result from the projection of distal objecs on to the retina. The diferent timing models rooted in this tradition have consequently relied on combining visual angle and its rate of expansion in diferent ways with tau being the most well-known solution for TTC...